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Longitudinal Spin at RHIC. Cameron McKinney. 29 th Winter Workshop on Nuclear Dynamics February 7, 2013. Introduction: Longitudinal Spin at RHIC. From the RHIC Spin white paper (2012 ):

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Longitudinal spin at rhic

Longitudinal Spin at RHIC

Cameron McKinney

29th Winter Workshop on Nuclear Dynamics

February 7, 2013


Introduction longitudinal spin at rhic

Introduction: Longitudinal Spin at RHIC

From the RHIC Spin white paper (2012):

Helicityparton density functions (PDFs) carry vital information on the extent to which quarks and gluons with a given momentum fraction x have their spins aligned with the spin direction of a fast moving nucleon in a helicityeigenstate. The corresponding integrals over all x relate to one of the most fundamental, but not yet satisfactorily answered questions in hadronic physics: how is the spin of the proton distributed among its constituents?

Proton Momentum

Proton Spin

Helicity

∆q(x,Q2)

∆g(x,Q2)

, where superscript +(-)

indicates parton spin aligned (anti-aligned) with proton spin

Cameron McKinney


Introduction longitudinal spin at rhic1

Proton spin:

Introduction: Longitudinal Spin at RHIC

Where does the proton’s spin of ½ come from?

}

RHIC longitudinal spin aims: ΔG and sea quark contribution to ΔΣ

Cameron McKinney


Outline

Outline

  • ΔG at RHIC

    • Accessing ΔG with double longitudinal spin asymmetries, ALL

    • Measuring ALL at RHIC

    • ΔG from ALL: Global analysis (by DSSV) with RHIC data

      • Impact of recent results from PHENIX+STAR

      • Next steps

  • Sea quark polarization at RHIC: the W program

    • Physics motivation: sea-quark polarization from ALW

    • Recent ALW results from STAR and PHENIX

    • Contribution of current and future data to DSSV global analysis

3

Cameron McKinney


Probing helicity structure in polarized pp collisions

Probing Helicity Structure in Polarized pp Collisions

Factorization: can break down cross section into pQCD-calculable hard scattering and pQCD-incalculable PDFs and fragmentation functions

pp  hX

Double longitudinal spin asymmetry is sensitive to Δgand Δq

4

Cameron McKinney


Measuring a ll at rhic

Measuring ALL at RHIC

  • ALLis measured by determining difference in particle yields between ++ and +- crossings (with an additional factor to normalize luminosities for crossing types)

  • Bunch spinpatterns include ++,+-, -+, and -- crossings in each fill

  • N is the yield of the final state measured

    • e.g. jets, di-hadron or di-jet states

Cameron McKinney


Measuring a ll at rhic a ll for inclusive jets at star

20

10

Measuring ALL at RHIC: ALLfor Inclusive Jets at STAR

STAR Run 6 inclusive jet

Mid-rapidity, s=200 GeV

PRD 86, 032006 (2012)

Process Fraction

pT [GeV]

  • STAR inclusive jet measurements at mid-rapidity have most statistics where qg processes dominatesensitive to sign of Δg

Good discriminative power between calculations with different assumptions for G

6

Cameron McKinney


Measuring a ll at rhic a ll for inclusive 0 at phenix

Measuring ALL at RHIC: ALLfor Inclusive 0at PHENIX

PHENIX Run5+6 √s = 200 GeV: PRL103, 012003

Process Fraction

  • PHENIX ALL for inclusive π0 covers a scaled-down pT range compared to STAR—π0’s carry a fraction of jet momentum

  • Smallest statistical uncertainty where process fraction for gg ≈ qgweaker constraint on negative Δg, better constraints on positive Δg

7

Cameron McKinney


G from a ll qcd global analysis

ΔG from ALL: QCD Global Analysis

  • DSSV (de Florian, Sassot, Stratmann, Vogelsang): global NLO analysis including polarized data from inclusive DIS, SIDIS, and RHIC pp collisions

    • Phys.Rev.Lett.101:072001, 2008 and Phys.Rev.D80:034030,2009.

Inclusive DIS data: routinely used for PDF fits

Semi-inclusive DIS data: previously used only in DNS fit

flavor separation

First RHIC polarized pp data: first fit by DSSV

467 data points in total (10% from RHIC)

Cameron McKinney


G from a ll qcd global analysis1

ΔG from ALL: QCD Global Analysis

  • Methodology Overview:

    • Parameterize distributions for quarks and gluons

    • Impose additional physics-based constraints (e.g. )

    • Evolve distributions from the input scale to the various Q2 of experimental data

    • Find corresponding observables as a function of kinematic variable (pTfor pp, x for DIS)

    • Minimize of fit of calculated observables to data

Cameron McKinney


G from a ll qcd global analysis2

ΔG from ALL: QCD Global Analysis

  • Methodology Overview:

Parameterize distributions…

…calculate observables and fit to data

(STAR and PHENIX Run 5 + Run 6 data shown).

DSSV: Phys.Rev.Lett.101:072001, 2008

Cameron McKinney


G from a ll dssv results

ΔG from ALL: DSSV Results

Well-determined by DIS

Main constraints to sea quarks from SIDIS (and DIS for strange quark)

Best constraints for ΔG now provided by RHIC

de Florian, Sassot, Stratmann, Vogelsang

Phys.Rev.D80:034030,2009

Cameron McKinney


G from a ll run 9 a ll measurements at rhic

ΔG from ALL: Run 9 ALL Measurements at RHIC

STAR preliminary

  • Substantially larger figure of merit (P4L) from Run 9 than in all previous runs combined.

Cameron McKinney


G from a ll dssv with run 9 data

ΔG from ALL: DSSV with Run 9 Data

  • DSSV++ is a new, preliminary global analysis from the DSSV group that includes 2009 ALL measurements from PHENIX and STAR

  • First experimental evidence of non-zero gluon polarization in the RHIC range (0.05 < x< 0.2)!

Cameron McKinney


G from a ll dssv with run 9 data1

ΔG from ALL: DSSV with Run 9 Data

Cameron McKinney


G at rhic next steps

ΔG at RHIC: Next Steps

  • Large uncertainty still remains in both the shape of Δg(x) and its integral, particularly for small x region not yet accessed by RHIC data

  • RHIC will continue to improve constraints through the following:

    • Reduced statistical and systematic uncertainties for all ALL channels

    • Better handle on measured x through correlation measurements

    • Access lower x region through forward measurements and

Cameron McKinney


G at rhic next steps correlation measurements

ΔG at RHIC: Next Steps: Correlation Measurements

Measure two jets or jet tags to constrain event kinematics; provides data on shape of

STAR di-jet projections;

one jet at forward rapidity (1<<2) to push down x2

ALL for back-to-back ’s at mid-rapidity—more data needed!

Cameron McKinney


G at rhic next steps low x with the mpc in phenix

ΔG at RHIC: Next Steps: Low x with the MPC in PHENIX

Larger  smaller x2

MPC: 3.1<<3.9

Projections of cluster ALLwith Run 13 for 2009 DSSV best fitand Δg upper uncertainty band

First PHENIX forward measurement of ALL for merged EM clusters (~80% 0)

Cameron McKinney


G at rhic next next steps electron ion collider

ΔG at RHIC: Next Next Steps: Electron-Ion Collider

  • Proposed electron-ion collider could greatly enhance our knowledge of Δ𝑮 beyond current capabilities of RHIC

    • Polarization of both electron (~80%) and proton beam (70%)

    • Very high luminosity (~10 fb-1 used for projection below achievable in 1-2 months of running)

    • Broad coverage in Q2 and x allows precise determination of Δg(x) through scaling violation

-DSSV+

-w proj. EIC data

(~10 fb-1)

x

Cameron McKinney


Sea quark polarization w program at rhic

Sea Quark Polarization: W Program at RHIC

Previously constrained by SIDIS:

Large uncertainties from fragmentation functions and lack of data

  • Measurement of parity-violating W production at RHIC complements SIDIS data

    • Leptonic final stateno FF dependence

    • Large Q2 ~ MW2

    • W couples only to left-handed quarks and right-handed anti-quarksfixes quark helicity and flavor

Cameron McKinney


W program at rhic forward upgrades

W Program at RHIC: Forward Upgrades

  • Selecting kinematic ranges allows sensitivity to specific quark/anti-quark helicities; upgrades allow lepton measurements at forward rapidity

Forward Gem Tracker

  • Central (barrel) region (We , ||<1)

    • First data from 2009: PRL106, 062002 (2011)

  • Forward (endcap) region (We , 1<||<2) :

    • Forward tracker upgrade, first data in 2012

  • Central Arms (We , ||<0.35)

    • First data from 2009: PRL106, 062001 (2011)

  • Forward Arms (W , 1.2<||<2.4) :

    • Trigger upgraded, first data from 2011

RPC-1 North and RPC-3 North

20

Cameron McKinney


W program at rhic forward measurements of a l

W Program at RHIC: Forward Measurements of AL

  • First measurement of by PHENIX in 2011 (

(towards )

Cameron McKinney


W program at rhic forward measurements of a l1

W Program at RHIC: Forward Measurements of AL

  • STAR preliminary AL for Run 12 already has sizeable effect on DSSV fits

DSSV++ (includes STAR Run 12)

DSSV+

(DSSV with COMPASS)

Cameron McKinney


W program at rhic next steps

W Program at RHIC: Next Steps

  • Run 13 goal: finish W program by reaching total

Projections including expected data in 2013

Cameron McKinney


Summary

Summary

  • The PHENIX and STAR collaborations are making important contributions to our understanding of the helicity structure of the nucleon

  • ALL measurements provide best constraints to ΔG for QCD analyses

    • For the first time we see evidence of a non-zero gluon polarization

    • Large dataset from Run 13 at of 510 GeVwill lead to precise measurement of at 0.05 < x < 0.2

    • ALL for correlations and at forward rapidity will reduce uncertainties in the shape and integral of Δg(x) while broadening the coverage in x down to ~10-3

  • W program at RHIC will lead to substantial improvement in the understanding of the sea quark polarization in the near term with the expected statistics from Run 13

    • The STAR AL from Run 12 has already provided DSSV with a stronger constraint on the sea quark polarization

Cameron McKinney


Longitudinal spin at rhic

Backup

Cameron McKinney


Constraining x probing low x

Constraining x/probing low x

Fwd–Rapidity 3.1<|η| < 3.9, 500 GeV

Single

π0

Effect of higher COM energy

Di-π0

Cameron McKinney


Central region w e from run9

Central region: W  e from Run9

ALe+/e-

ALe+/e-

e+

e-

e-

e+

PHENIX: PRL106, 062001 (2011)

STAR: PRL106, 062002 (2011)

P=0.39 L=8.6/12 pb-1 in PHENIX/STAR

27

Cameron McKinney


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